The present page contains a
catalog
of models of irradiated accretion disks around pre-main sequence stars
by D'Alessio
et al. (1998,1999,2001).
Radial profiles of the detailed vertical structure and synthetic SEDs
can be browsed and downloaded from this catalog.

The present web page is
described
in detail in D'Alessio et al. (2004, click here for a pdf,
or gzipped
ps, format of the paper). Here we just mention
that the model includes the disk heating by stellar radiation
(considered
in a shorter wavelength regime respect to the disk own radiation
field),
viscous dissipation (using the prescription), and ionization by energetic
particles (cosmic rays and radioactive decay). The energy of the disk
model
is transported by radiation, convection and a turbulent flux. The
disk is assumed axisymmetric, with gas and dust well mixed. The opacity
is calculated taking into account both dust and gas. For the gas, the
populations
of selected molecules are calculated assuming LTE. For the dust, we
explore
different grain size distributions.